Evolution of brightness and magnetic features of young solar-type stars II: The young F8 star HIP 71933

Abstract The early, active history of our Sun is still not fully understood. Observations of the magnetic fields on active young solar-type stars allows us an insight into the early evolution of our Sun. Here we present Doppler and Zeeman Doppler images of the young late-F star HIP 71933 (HD 129181) at multiple epochs to add to the growing data about the evolution of magnetic cycles in solar-type stars. Spectroscopic data were obtained over seven epochs spanning ten years of observations, with two epochs including spectropolarimetric data. The brightness maps at all epochs show a consistent spot activity in a non-uniform ring at a latitude of approximately +60○ with no polar spot present in any epoch. The two magnetic field maps taken ∼2 years apart show a strong poloidal field configuration with most of the poloidal field energy in the dipolar configuration. The magnetic maps show no evidence of a polarity reversal. We were able to measure the differential rotation from one of the seven epochs using the brightness data finding a dΩ of 0.325 ± 0.01 rad d−1. The values for rotational period and differential rotation found for HIP 71933 are consistent with values found for other late-F or early-G stars. The dominant poloidal features and the limited spots at the pole are unusual for a rapidly rotating star but not unique.